The delay between solar EUV flare emission and ionospheric F-region response is under a minute and shorter for stronger flares.
Confirming geomagnetic Sfe by means of a solar flare detector based on GNSS
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Investigating a Characteristic Time Lag in the Ionospheric F-region's Response to Solar Flares
The delay between solar EUV flare emission and ionospheric F-region response is under a minute and shorter for stronger flares.